Some results from small stars of nuclear emulsion at 24 GeV
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Published:1980-11-01
Issue:11
Volume:58
Page:1580-1584
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ISSN:0008-4204
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Container-title:Canadian Journal of Physics
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language:fr
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Short-container-title:Can. J. Phys.
Author:
Ahmad I.,Khan A. R.,Ahsan M. Z.,Zafar M.,Irfan M.,Shafi M.
Abstract
The analysis of 400 stars with 2 ≤ Nh ≤ 7 has been performed to investigate the emission characteristics of protons, deuterons, tritons, and slow pions produced in interactions of 24 GeV/c protons in nuclear emulsion. The [Formula: see text] and [Formula: see text] distributions of these particles have been experimentally investigated. The dependence of [Formula: see text] and [Formula: see text] on the shower multiplicity, the angle of emission, and mass of the particles has been studied.
Publisher
Canadian Science Publishing
Subject
General Physics and Astronomy
Cited by
1 articles.
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